Numerical Methods for the Einstein Equations in Null Quasi-Spherical Coordinates

DOI10.1137/S1064827599356171zbMath0973.83004arXivgr-qc/9904045OpenAlexW2139680668MaRDI QIDQ4509864

Andrew H. Norton, Robert Bartnik

Publication date: 19 October 2000

Published in: SIAM Journal on Scientific Computing (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9904045

zbMATH Keywords

spherical harmonicsblack holeEinstein equationsconvolution splinepreconditioned elliptic system

Mathematics Subject Classification ID

Numerical computation using splines (65D07) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Spectral, collocation and related methods for initial value and initial-boundary value problems involving PDEs (65M70) Method of lines for initial value and initial-boundary value problems involving PDEs (65M20) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Related Items (9)

Extraction of gravitational waves in numerical relativity ⋮ Characteristic evolution and matching ⋮ Characteristic evolution and matching ⋮ Computing with Functions in Spherical and Polar Geometries I. The Sphere ⋮ Characteristic evolution and matching ⋮ Spectral methods for numerical relativity ⋮ Characteristic evolution and matching ⋮ NEW METHOD FOR CHARACTERISTIC EVOLUTIONS IN NUMERICAL RELATIVITY ⋮ Continuum and discrete initial-boundary value problems and Einstein's field equations

Uses Software

• REDUCE

This page was built for publication: Numerical Methods for the Einstein Equations in Null Quasi-Spherical Coordinates